PMAS optical integral field spectroscopy of luminous infrared galaxies - I. The atlas

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Volume 506 / No 3 (November II 2009)

A&A, 506 3 (2009) 1541-1562

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Table 1:

Log of the PMAS observations.
Galaxy	Dist	$\log L_{\rm IR}$	Date	Galaxy $t_{\rm int}$	Sky $t_{\rm int}$	Airmass	Seeing	Conditions
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)
NGC 23	59.6	11.05	7 Nov. 2005	$3 \times 1000$	1000	1.06	1.0-1.2	P
MCG +12-02-001	64.3	11.44	18 Dec. 2006	$4 \times 800$	1000	1.47	1.7	NP
UGC 1845	62.0	11.07	8 Nov. 2005	$3 \times 900$	900	1.05	1.4-2.0	NP
NGC 2388	57.8	11.23:	7 Nov. 2005	$3 \times 1000$	1000	1.04	1.3-1.1	P
MCG +02-20-003	67.6	11.08:	17 Dec. 2006	$4 \times 800$	1000	1.60	1.2	NP
IC 860	59.1	11.17:	30 May 2006	$4 \times 800$	1000	1.03	1.7	NP
NGC 5936	60.8	11.07	30 May 2006	$4 \times 800$	1000	1.17	1.5	NP
NGC 6701	56.6	11.05	30 May 2006	$1\times400 + 4\times 600$	800	1.09	1.3	NP
NGC 7469	65.2	11.59	8 Nov. 2005	$3 \times 900$	900	1.15	1.2	NP
NGC 7591	65.5	11.05	8 Nov. 2005	$3 \times 1000$	1000	1.32	1.1-1.2	NP
NGC 7771-E	57.1	11.34	7 Nov. 2005	$2\times 500 + 2\times 1000$	1000	1.15	0.8	P
NGC 7771-W	$\cdots$	$\cdots$	7 Nov. 2005	$3 \times 1000$	1000	1.06	0.8	P

Notes. - Column (1): galaxy. For NGC 7771 we took two different pointings to cover the approximate central $28\hbox {$^{\prime \prime }$ }\times 16\hbox {$^{\prime \prime }$ }$ region of the galaxy, as explained in the text. Columns (2) and (3): distance (in Mpc) and IR luminosity (in $L_\odot$ ) taken from Sanders et al. (2003) for the IRAS RBGS. Column (4): date of the observations. Column (5): integration time (in seconds) of the galaxy observations after discarding bad data sets. Column (6): integration time (in seconds) of the sky observations. Column (7): airmass at the beginning of the observation. Column (8): typical seeing conditions (in arcseconds) of the observations. If two values of the seeing are given they correspond to the beginning and the end of the observations. Column (9): observing conditions. P: Photometric. NP: Non-photometric.

Source LaTeX | All tables | In the text

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